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Implications of Low Neutron Star Merger Rates for Gamma-Ray Bursts, r-process Production, and Galactic Double Neutron Stars

  • Authors: Maya Fishbach, Alexander P. Ji, Wen-fai Fong, Tom Y. Wu, Jillian C. Rastinejad, Aditya Vijaykumar, Hsin-Yu Chen

Maya Fishbach et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 1.

Inferred BNS merger rate as a function of time, compared to the rates of SGRBs, MW DNS systems, and the rate required to explain the MW r-process mass. The GWTC-1 and GWTC-3 inferred rates show the union of 90% error bars over different posteriors (that assume different mass distributions), so we represent them as shaded blue rectangles. The GWTC-4 posterior inferred in this work is shown as a violin. The dashed, unfilled blue rectangles show the approximate 90% credible intervals on the BNS rate at the end of O4 if there are 0 new BNS or 1 new BNS detected in O4 once the data are fully analyzed.

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